Shrivastava, A.K. and Ishwar, B. (1983) Equations of Motion of the Restricted Problem of Three Bodies with Variable Mass. Celestial Mechanics and Dynamical Astronomy, 30, 323-328.
ttps://doi.org/10.1007/BF01232197

has been cited by the following article:

• TITLE: Existence of Equilibrium Points in the R3BP with Variable Mass When the Smaller Primary is an Oblate Spheroid

  AUTHORS: M. R. Hassan, Sweta Kumari, Md. Aminul Hassan

  KEYWORDS: Restricted Three-Body Problem, Jean’s Law, Space-Time Transformation, Oblateness, Equilibrium Points, Surface of Zero-Velocity

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.7 No.2, April 12, 2017

  ABSTRACT: The paper deals with the existence of equilibrium points in the restricted three-body problem when the smaller primary is an oblate spheroid and the infinitesimal body is of variable mass. Following the method of small parameters; the co-ordinates of collinear equilibrium points have been calculated, whereas the co-ordinates of triangular equilibrium points are established by classical method. On studying the surface of zero-velocity curves, it is found that the mass reduction factor has very minor effect on the location of the equilibrium points; whereas the oblateness parameter of the smaller primary has a significant role on the existence of equilibrium points.